{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1993:V2C4OVIZCJV6AYMLOBQJD2WUAF","short_pith_number":"pith:V2C4OVIZ","schema_version":"1.0","canonical_sha256":"ae85c75519126be0618b706091ead401717a4cee0d9eac12b1496b22845d1eae","source":{"kind":"arxiv","id":"hep-ph/9303313","version":1},"attestation_state":"computed","paper":{"title":"Axion Miniclusters and Bose Stars","license":"","headline":"","cross_cats":["astro-ph","gr-qc"],"primary_cat":"hep-ph","authors_text":"Edward W. Kolb, Igor I. Tkachev","submitted_at":"1993-03-29T22:24:17Z","abstract_excerpt":"Evolution of inhomogeneities in the axion field around the QCD epoch is studied numerically, including for the first time important non-linear effects. It is found that perturbations on scales corresponding to causally disconnected regions at $T \\sim 1 \\, {\\rm GeV}$ can lead to very dense axion clumps, with present density $\\rho_a \\ga 10^{-8}\\,{\\rm g \\, cm^{-3}}$. This is high enough for the collisional $2a \\rightarrow 2a$ process to lead to Bose--Einstein relaxation in the gravitationally bound clumps of axions, forming Bose stars."},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"hep-ph/9303313","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"1993-03-29T22:24:17Z","cross_cats_sorted":["astro-ph","gr-qc"],"title_canon_sha256":"82d5ae888948d66419acd3edd7424c19a1dc74b1e8b63e426e9868bd30d24966","abstract_canon_sha256":"dfe504267174b19b8e5378a423319cc404dc8a452f24383f4637782606503723"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:55:45.787905Z","signature_b64":"tm1DxmnrJW7znCoAeatRk74iqwdkAc8mklHHRfpEfTrPb7VcPM4MncK+nyOv8llgQ/xNB1y5bXo6Y/KRSI0XCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ae85c75519126be0618b706091ead401717a4cee0d9eac12b1496b22845d1eae","last_reissued_at":"2026-07-04T15:55:45.787556Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:55:45.787556Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Axion Miniclusters and Bose Stars","license":"","headline":"","cross_cats":["astro-ph","gr-qc"],"primary_cat":"hep-ph","authors_text":"Edward W. Kolb, Igor I. Tkachev","submitted_at":"1993-03-29T22:24:17Z","abstract_excerpt":"Evolution of inhomogeneities in the axion field around the QCD epoch is studied numerically, including for the first time important non-linear effects. It is found that perturbations on scales corresponding to causally disconnected regions at $T \\sim 1 \\, {\\rm GeV}$ can lead to very dense axion clumps, with present density $\\rho_a \\ga 10^{-8}\\,{\\rm g \\, cm^{-3}}$. This is high enough for the collisional $2a \\rightarrow 2a$ process to lead to Bose--Einstein relaxation in the gravitationally bound clumps of axions, forming Bose stars."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9303313","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/hep-ph/9303313/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"hep-ph/9303313","created_at":"2026-07-04T15:55:45.787618+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/9303313v1","created_at":"2026-07-04T15:55:45.787618+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/9303313","created_at":"2026-07-04T15:55:45.787618+00:00"},{"alias_kind":"pith_short_12","alias_value":"V2C4OVIZCJV6","created_at":"2026-07-04T15:55:45.787618+00:00"},{"alias_kind":"pith_short_16","alias_value":"V2C4OVIZCJV6AYML","created_at":"2026-07-04T15:55:45.787618+00:00"},{"alias_kind":"pith_short_8","alias_value":"V2C4OVIZ","created_at":"2026-07-04T15:55:45.787618+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":12,"internal_anchor_count":10,"sample":[{"citing_arxiv_id":"2607.05278","citing_title":"Spin Polarization of Proca Stars Formed by Gravitational Bose--Einstein Condensation","ref_index":25,"is_internal_anchor":true},{"citing_arxiv_id":"2606.19439","citing_title":"From Rags to Jeans: Axion Miniclusters from Early matter domination","ref_index":23,"is_internal_anchor":true},{"citing_arxiv_id":"2607.01333","citing_title":"Axion Misalignment Across First-Order Phase Transitions","ref_index":57,"is_internal_anchor":true},{"citing_arxiv_id":"2606.06484","citing_title":"Phenomenology of Inflaton-Driven Early QCD Confinement and Solution to Axion Isocurvature Problem","ref_index":13,"is_internal_anchor":true},{"citing_arxiv_id":"2605.28005","citing_title":"Transient axion streams from disrupted miniclusters","ref_index":10,"is_internal_anchor":true},{"citing_arxiv_id":"2606.01103","citing_title":"Self-gravitating quantum stars with a globally relevant Bohm potential","ref_index":105,"is_internal_anchor":true},{"citing_arxiv_id":"2510.15046","citing_title":"Multi-species Dark Matter with Warmth and Randomness","ref_index":32,"is_internal_anchor":true},{"citing_arxiv_id":"2510.17977","citing_title":"Growth of Structure in Multi-species Wave Dark Matter","ref_index":30,"is_internal_anchor":true},{"citing_arxiv_id":"2509.17059","citing_title":"Axions as Dark Matter, Dark Energy, and Dark Radiation","ref_index":132,"is_internal_anchor":true},{"citing_arxiv_id":"2601.07670","citing_title":"Tachyonic gravitational dark matter production after inflation","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2604.06082","citing_title":"Hunting Dark Matter with the Einstein Telescope","ref_index":47,"is_internal_anchor":false},{"citing_arxiv_id":"2604.17083","citing_title":"Dark ages bounds on non-accreting massive compact halo objects","ref_index":33,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/V2C4OVIZCJV6AYMLOBQJD2WUAF","json":"https://pith.science/pith/V2C4OVIZCJV6AYMLOBQJD2WUAF.json","graph_json":"https://pith.science/api/pith-number/V2C4OVIZCJV6AYMLOBQJD2WUAF/graph.json","events_json":"https://pith.science/api/pith-number/V2C4OVIZCJV6AYMLOBQJD2WUAF/events.json","paper":"https://pith.science/paper/V2C4OVIZ"},"agent_actions":{"view_html":"https://pith.science/pith/V2C4OVIZCJV6AYMLOBQJD2WUAF","download_json":"https://pith.science/pith/V2C4OVIZCJV6AYMLOBQJD2WUAF.json","view_paper":"https://pith.science/paper/V2C4OVIZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/9303313&json=true","fetch_graph":"https://pith.science/api/pith-number/V2C4OVIZCJV6AYMLOBQJD2WUAF/graph.json","fetch_events":"https://pith.science/api/pith-number/V2C4OVIZCJV6AYMLOBQJD2WUAF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/V2C4OVIZCJV6AYMLOBQJD2WUAF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/V2C4OVIZCJV6AYMLOBQJD2WUAF/action/storage_attestation","attest_author":"https://pith.science/pith/V2C4OVIZCJV6AYMLOBQJD2WUAF/action/author_attestation","sign_citation":"https://pith.science/pith/V2C4OVIZCJV6AYMLOBQJD2WUAF/action/citation_signature","submit_replication":"https://pith.science/pith/V2C4OVIZCJV6AYMLOBQJD2WUAF/action/replication_record"}},"created_at":"2026-07-04T15:55:45.787618+00:00","updated_at":"2026-07-04T15:55:45.787618+00:00"}